Abstract
Series expansion of the two-spin correlation functions is obtained in the context of the hybrid quantum-classical method of simulation of high-temperature spin dynamics. The resulting series are compared with the corresponding series for the exact correlation functions obtained from purely quantum dynamics.
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Acknowledgements
I would like to thank Professor Boris Fine for the invaluable scientific advice. This work was supported by a grant of the Russian Science Foundation (Project No. 17-12-01587).
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Appendix: Infinite-Temperature Correlators of Arbitrary Order
Appendix: Infinite-Temperature Correlators of Arbitrary Order
In the calculation of the series expansion of the correlation functions in the hybrid case, one encounters the correlators of the form:
where \([\cdots ]_\psi\) denotes the average over the infinite-temperature ensemble of normalized uniformly distributed wave-functions \(|\psi \rangle\). If we represent the wave-function
in terms of some full orthonormal basis \({|k\rangle }\), we can reformulate Eq. (49) as
where
Given a particular choice of orthonormal basis in representation (50), the correlators for arbitrary sets of observables are completely determined by the matrix elements of observables and by the tensors:
Since the distribution of wave functions describing infinite temperature is invariant with respect to unitary transformations, the choice of the orthonormal basis \(|k\rangle\) in representation (50) is arbitrary. As a consequence, the form of the tensors \(F^{i_1,i_2,\dotsc ,i_n}_{j_1,j_2,\dotsc ,j_n}\) is identical irrespective of this choice.
In order to deduce the form of the tensors \(F^{i_1,i_2,\dotsc ,i_n}_{j_1,j_2,\dotsc ,j_n}\) of arbitrary order, it is convenient to recast the Hilbert space average \([\cdots ]_{\psi }\) as a multidimensional integral over the expansion coefficients \(a_i\) in representation (50):
where \(\delta (\cdots )\) is the Dirac delta-function. Here the measure of integration \(\mathrm{d}\mu\) is defined in terms of the decomplexification of the Hilbert space:
The denominator of Eq. (54) is the area \(A_{2D-1}\) of the \((2D-1)\)-dimensional unit hypersphere.
In order to evaluate the right-hand side of Eq. (54), let us introduce an auxiliary multidimensional integral:
On the one hand, it is a simple Gaussian integral and can be evaluated in the closed form with the use of the Wick’s theorem (see, for example, [21, Chapter 1]) as
where the summation is performed over all the permutations P of n indices \(\{j_1,j_2,\dotsc ,j_n\}\). On the other hand, we can split the integration into the integration over the surface of the \((2D-1)\)-dimensional hyper-sphere of radius r with the subsequent integration over the radius of that hypersphere:
Here we have used the fact that
In Eq. (58),
where \(\varGamma (x)\) is the Euler’s gamma function, and
for odd n. Thus,
Substituting Eq. (62) into Eq. (58) and comparing the result with Eq. (57), we, finally, get
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Starkov, G.A. Time Series Analysis of the Hybrid Quantum-Classical Method of Simulation of High-Temperature Spin Dynamics. Appl Magn Reson 52, 843–858 (2021). https://doi.org/10.1007/s00723-021-01355-w
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DOI: https://doi.org/10.1007/s00723-021-01355-w